717 citations · 19.6k across the 253 of their papers we have counts for
254 papers
Resumming Kerr Quasinormal-Mode Frequencies: Accuracy and Breakdown Near Extremality
Jierui Hu, Kent Yagi, Nicolas Yunes
Kerr black-hole quasinormal modes are usually computed with numerical methods, but analytic approximations remain useful for identifying the physics that controls different parts o…
Gravitational waves of quasi-circular, inspiraling black hole binaries in an ultralight vector dark-matter environment
Tomás Ferreira Chase, Diana López Nacir, Nicolás Yunes
The gravitational waves emitted by massive black hole binaries can be affected by a variety of environmental effects, which, if detected, could inform astrophysics and cosmology. W…
Constraining dark-sector effects using gravitational waves from compact binary inspirals
Caroline B. Owen, Alexandria Tucker, Yonatan Kahn +1
Gravitational wave observations are a powerful tool to constrain fundamental physics. This work considers dark matter that carries charge under a dark abelian massive vector field.…
Better early than never: A new test for superluminal gravitational wave polarizations
Kristen Schumacher, Colm Talbot, Daniel E. Holz +1
In some beyond-Einstein theories of gravity, gravitational waves can contain up to six polarizations, which are allowed to propagate at different speeds faster than light. These di…
Improved Analytic Love-C Relations for Neutron Stars
Tristen Lowrey, Kent Yagi, Nicolás Yunes
Precise measurements of neutron star observables (such as mass and radius) allow one to constrain the equations of state for supranuclear matter and develop a stronger understandin…
Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
Rohit S. Chandramouli, Kaitlyn Prokup, Emanuele Berti +1
We study the robustness of parametrized post-Einsteinian (ppE) tests of General Relativity (GR) with gravitational waves, due to waveform inaccuracy. In particular, we determine th…